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Theoretical gamma-ray astrophysics research conducted in the Laboratory for High-Energy Astrophysics concerns astrophysical processes that produce emission at gamma-ray energies. This research attempts to answer fundamental questions such as the origin, structure, and evolution of the Universe; the nature of compact objects; the origin of the cosmic rays; and the structure and evolution of the galaxy. Research is performed on gamma-ray line and continuum production mechanisms, on physical processes in strong magnetic fields, on the physics of electron-positron pair plasmas, and on radiation transfer in the gamma-ray regime. These physical processes are applied to models of compact sources, including active galactic nuclei, the galactic center, galactic gamma-ray sources, pulsars, and gamma-ray bursters. They are also applied to diffuse sources of gamma-rays, including the galaxy and young supernova remnants. Gamma-ray tests for the nature of dark matter are also proposed. Applicants are encouraged to participate in the above research or to initiate related projects. Gamma-ray tests of special relativity, as well as tests of proposed quantum gravity effects on high energy gamma-ray processes are also explored.
Location:
Goddard Space Flight Center
Greenbelt, Maryland
Field of Science:Astrophysics
Advisors:
Tonia Venters
tonia.m.venters@nasa.gov
301-614-5546
Demosthenes Kazanas
Demos.Kazanas-1@nasa.gov
301-286-7680
Zaven Arzoumanian
zaven.arzoumanian-1@nasa.gov
(301) 286-2547
Tyler M. Parsotan
tyler.parsotan@nasa.gov
301-286-4678
Applications with citizens from Designated Countries will not be accepted at this time, unless they are Legal Permanent Residents of the United States. A complete list of Designated Countries can be found at: https://www.nasa.gov/oiir/export-control.
Eligibility is currently open to:
Full Time
$79k-102k (estimate)
09/26/2023
05/30/2024
ssc.nasa.gov
Stennis Space Center, MS
100 - 200